VISIR/VLT and VLA joint imaging analysis of the circumstellar nebula around IRAS~18576+0341
arXiv:1008.0997 · doi:10.1088/0004-637X/721/2/1404
Abstract
High spatial and sensitivity images of the Luminous Blue Variable IRAS 18576+0341 were obtained using the mid infrared imager VISIR at the Very Large Telescope and the Very Large Array interferometer. The resulting mid-infrared continuum maps show a similar clumpy and approximately circular symmetric nebula, which contrasts sharply with the asymmetry that characterizes the ionized component of the envelope, as evidenced from the radio and [Ne II] line images obtained with comparable spatial resolution. In particular, there is excellent overall agreement between the 12.8 micron map and the radio images, consistent with free-free emission from circumstellar ionized material surrounding a central stellar wind. The color temperature and optical depth maps obtained from mid-infrared images show only slight fluctuations, suggesting quite uniform dust characteristics over the dust shell. We explore various possibilities to understand the cause of the different morphology of the dusty and gaseous component of the circumstellar envelope which are compatible with the observations.
arXiv comment26 pages, 8 figures. Accepted for publication in The Astrophysical Journal
References in corpus (14)
- The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
- On the role of continuum-driven eruptions in the evolution of very massive stars and Population III stars
- Luminous Blue Variables as the progenitors of supernovae with quasi-periodic radio modulations
- A Hidden Population of Massive Stars with Circumstellar Shells Discovered with the Spitzer Space Telescope
- Grain size distributions and photo-electric heating in ionized media
- Infrared [Fe II] emission from P Cygni's nebula: Atomic data, mass, kinematics, and the 1600 A.D. outburst
- Bolometric luminosity variations in the Luminous Blue Variable AFGL2298
- Stellar Winds and Embedded Star Formation in the Galactic Center Quintuplet and Arches Clusters: Multifrequency Radio Observations
- Doppler tomography of the Little Homunculus: High resolution spectra of [Fe II] 16435 around Eta Carinae
- Detection of a massive dust shell around the Type II supernova SN 2002hh
- Discovery of an Extended Dust Emission around IRAS 18576+0341 (AFGL 2298) at 10.3 and 18.0 microns: a New Luminous Blue Variable Candidate?
- Radio Detections of Stellar Winds from the Pistol Star and Other Stars in the Galactic Center Quintuplet Cluster
- The dusty Nebula surrounding HR Car: a Spitzer view
- Multiple shells around G79.29+0.46 revealed from near-IR to millimeter data
Cited by in corpus (11)
- The Astrophysical Implications of Dust Formation During The Eruptions of Hot, Massive Stars
- Search for OB stars running away from young star clusters. II. The NGC 6357 star-forming region
- Herschel/PACS observations of the 69 band of crystalline olivine around evolved stars
- Exploring the multifaceted circumstellar environment of the Luminous Blue Variable HR Carinae
- New ATCA, ALMA and VISIR observations of the candidate LBV SK-67266 (S61): the nebular mass from modelling 3D density distributions
- The Luminous Blue Variable RMC127 as seen with ALMA and ATCA
- A massive nebula around the Luminous Blue Variable star RMC143 revealed by ALMA
- The contribution by luminous blue variable stars to the dust content of the Magellanic Clouds
- MeerKAT reveals a ghostly thermal radio ring towards the Galactic Centre
- VISIR-VLT high resolution study of the extended emission of four obscured post-AGB candidates
- The rich molecular environment of the luminous blue variable star AFGL 2298